Ionized gases from the nucleus of a spiral or irregular galaxy

Details Ionized gases from the nucleus of a spiral or irregular galaxy Ionized gases from the nucleus of a spiral or irregular galaxy

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jrasc..81..128v&link_type=abstract

Journal of the Royal Astronomical Society of Canada (ISSN 0035-872X), vol. 81, Aug. 1987, p. 128-141. In French.

Other

Galactic Nuclei, Hydrogen Clouds, Interstellar Gas, Ionized Gases, Irregular Galaxies, Spiral Galaxies, Abundance, Galactic Structure, Mass Distribution, Molecular Clouds, Star Formation Rate

Scientific paper

In the disk of a spiral galaxy or outside of the nucleus of an irregular galaxy, the morphology of hot ionised gaseous regions (H II regions) can take many shapes: champagne or blister, bubble or half-bubble, giant complex, etc. Two basic types of internal turbulences in the H II regions have been proposed: "ordered" (champagne, wind, etc.) and "random" (relative motions, self-gravitation, differential rotation, etc.). Other deductions have been obtained from the observations, regarding the luminosity and the rate of star formation.

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